Step 1: Energy change due to relativistic motion.
The total energy \( E \) of a moving particle is given by:
\[
E = \gamma m c^2
\]
where \( \gamma = \frac{1}{\sqrt{1 - \frac{v^2}{c^2}}} \) is the Lorentz factor, \( v \) is the velocity of the electron, and \( c \) is the speed of light.
Step 2: Calculate the change in energy.
For an electron accelerated to \( 0.5c \), we calculate \( \gamma \):
\[
\gamma = \frac{1}{\sqrt{1 - \frac{(0.5c)^2}{c^2}}} = \frac{1}{\sqrt{1 - 0.25}} = \frac{1}{\sqrt{0.75}} \approx 1.1547
\]
The total energy is:
\[
E = \gamma \times 0.511 \, \text{MeV} = 1.1547 \times 0.511 = 0.590 \, \text{MeV}
\]
Thus, the change in energy is:
\[
\Delta E = E - E_0 = 0.590 \, \text{MeV} - 0.511 \, \text{MeV} = 0.079 \, \text{MeV}
\]